Coupling relationship between reservoir diagenesis and hydrocarbon accumulation in Lower Cretaceous Yingcheng Formation of Dongling,Changling fault depression,Songliao Basin,Northeast China     

《China Geology》2020,3(2):247-261

The Lower Cretaceous Yingcheng Formation in the southern Songliao Basin is the typical tight oil sandstone in China. In order to better predict the petrophysical properties of the tight sandstone reservoirs in the Lower Cretaceous Yingcheng Formation, Songliao Basin, Northeast China, the diagenesis and porosity evolution was investigated using a suite of petrographic and geochemical techniques including thin section analysis, scanning electron microscopy, mercury intrusion and fluid inclusion analysis, on a set of selected tight sandstone samples. Combined with the histories of burial evolution, organic matter thermal evolution and hydrocarbon charge, the matching relationship between reservoir porosity evolution and hydrocarbon accumulation history is analyzed. The result showed that the tight sandstone reservoirs characterized of being controlled by deposition, predominated by compaction, improved by dissolution and enhanced by cementation. The hydrocarbon accumulation period was investigated using a suite of hydrocarbon generation and expulsion history, microfluorescence determination and temperature measurement technology. According to the homogenization temperature of the inclusions and the history of burial evolution, Yingcheng Formation has mainly two phases hydrocarbon accumulation. The first phase of oil and gas is charged before the reservoir is tightened, the oil and gas generated by Shahezi source rocks enter the sand body of Yingcheng Formation, influenced by the carrying capability of sand conducting layer, oil and gas is mainly conducted by the better properties and higher connectivity sand body and enriched in the east, which belongs to the type of densification after hydrocarbon accumulation. The second phase of oil and gas charge after densification, which belongs to the type of densification before the hydrocarbon accumulation.  相似文献   

不同非感应起电及感应起电参数化方案对青海东部一次雷暴云电荷结构影响的数值模拟研究          下载免费PDF全文

李江林  余晔  李万莉  李亚珺 《地球物理学报》2019,62(7):2366-2381

本研究利用加入起电、放电参数化方案的数值模式（Weather Research and Forecasting Model（Version 3.7.1），WRF3.7.1_ELEC），通过设计五组不同非感应起电及感应起电参数化方案敏感性试验，对发生在青藏高原东北部青海大通地区的一次雷暴过程进行模拟研究，对比分析了不同非感应起电机制及感应起电机制对雷暴云电荷结构的影响.结果表明：在雷暴云发展旺盛阶段，Saunders（S91）、Riming Rate（RR）、和Saunders和Peck（SP98）三种非感应起电方案模拟的雷暴云最低层均为负电荷区，而混合方案（Brooks and SP98，BSP）模拟的雷暴云最低层为正电荷区，主电荷区自下而上为"+-+-"排列的四层电荷结构.与甚高频辐射源定位法推算的结果对比，BSP方案模拟的本次高原雷暴云电荷结构更接近实际情况；几种不同非感应起电方案模拟的主电荷区外围与主电荷区电荷结构不同，说明在雷暴发展的不同阶段雷暴云的电荷结构是不同的；几种非感应起电方案模拟的电荷结构不尽相同，主要是由于霰、冰和雪粒子在不同高度所带电荷的极性及电量的大小不同，霰粒子的电荷密度对低层的影响较大，冰粒子和雪粒子的电荷密度对中上层的影响较大；加入感应起电机制后，雷暴云电荷结构分布几乎没有变化，但能使雷暴云发展旺盛阶段低层和中层的正负电荷区电荷密度有所加强.  相似文献   

Impact of the Vertical Velocity Field on Charging Processes and Charge Separation in a Simulated Thunderstorm          下载免费PDF全文

WANG Fei  ZHANG Yijun  ZHENG Dong  XU Liangtao 《Acta Meteorologica Sinica》2015,29(2):328-343

A three-dimensional(3D) charging-discharging cloud resolution model was used to investigate the impact of the vertical velocity field on the charging processes and the formation of charge structure in a strong thunderstorm. The distribution and evolution of ice particle content and charges on ice particles were analyzed in different vertical velocity fields. The results show that the ice particles in the vertical velocity range from 1 to 5 m s-1obtained the most charge through charging processes during the lifetime of the thunderstorm. The magnitude of the charges could reach 1014 n C. Before the beginning of lightning activity,the charges produced in updraft region 2(updraft speed 13 m s-1) and updraft region 1(updraft speed between 5 and 13 m s-1) were relatively significant. The magnitudes of charge reached 1013 n C, which clearly impacted upon the early lightning activity. The vertical velocity conditions in the quasi-steady region(updraft speed between –1 and 1 m s-1) were the most conducive for charge separation on ice particles on different scales. Accordingly, a net charge structure always appeared in the quasi-steady and adjacent regions. Based on the results, a conceptual model of ice particle charging, charge separation, and charge structure formation in the flow field was constructed. The model helps to explain observations of the"lightning hole" phenomenon.  相似文献   

Critical conditions for natural gas charging and delineation of effective gas source rocks for tight sandstone reservoirs     

Fujie Jiang  Xiongqi Pang  Fengtao Guo  Jigang Guo 《Geological Journal》2016,51(1):113-124

Although it has been shown that the potential of tight‐sand gas resources is large, the research into the mechanisms of hydrocarbon charging of tight sandstone reservoirs has been relatively sparse. Researchers have found that there is a force balance during hydrocarbon charging, but discriminant models still have not been established. Based on the force balance conditions observed during gas migration from source rocks to tight sandstone reservoirs, a calculation formula was established. A formula for identifying effective source rocks was developed with the gas expulsion intensity as the discrimination parameter. The critical gas expulsion intensity under conditions of various burial depths, temperatures, and pressures can be obtained using the calculation formula. This method was applied in the Jurassic tight sandstone reservoirs of the eastern Kuqa Depression, Tarim Basin, and it was calculated that the critical expulsion intensity range from 6.05 × 10⁸ m³/km² to 10.07 × 10⁸ m³/km². The critical gas charging force first increases with depth and later decreases with greater depths. The distribution range of effective gas source rocks and total expelled gas volume can be determined based on this threshold. This method provides new insight into and method for predicting favourable tight‐sand gas‐bearing regions and estimating their resource potentials. Copyright © 2014 John Wiley & Sons, Ltd.  相似文献   

基于贝叶斯方法的深层充电效应风险模型评估          下载免费PDF全文

李程  陈东 《地球物理学报》2019,62(6):1991-2000

高能电子穿透航天器并在其内部沉积电荷从而引发深层充电效应,是导致卫星故障的重要因素之一.为了评估深层充电效应诱发卫星异常的风险,本文基于贝叶斯方法,使用一颗地球同步轨道卫星的异常数据和GOES-8卫星的电子通量探测数据,计算了不同能量阈值及累积时间的电子注量、不同卫星配置下模拟仿真的沉积电荷,并分别与卫星异常建立一系列概率风险模型.本文从模型中随机抽样得到模拟异常,并与实测异常构造混淆矩阵以评估模型拟合优度,结果表明1.0MeV电子3日累积注量-卫星异常概率风险模型为该卫星最优模型.本文利用最优模型对该卫星深层充电效应风险进行了计算,在1.0MeV电子3日累积注量达到2.0×10~(10)cm~(-2)·sr~(-1)时,该卫星发生深层充电异常的平均后验概率为27%,且95%最小可信值为22%.根据最优模型,我们对该卫星最可能导致异常的部件的材料和结构等特征做出了推断.  相似文献   

Diagenesis and hydrocarbon emplacement in the Upper Triassic Yanchang Formation tight sandstones in the southern Ordos Basin,China     

H. Chen  C. Chen  W. Yin  Q. Zhang  R. Shi 《Australian Journal of Earth Sciences》2017,64(7):957-980

The Upper Triassic Yanchang Formation in the southern Ordos Basin is a tight sandstone but productive hydrocarbon exploration target. A variety of analyses, including thin-sections, cathodoluminescence (CL), scanning electron microscope (SEM), X-ray diffraction (XRD), fluorescence, isotope and fluid inclusion, have been used to analyse the reservoir petrology and diagenesis to understand the evolution of reservoir porosity. The sandstones are mostly feldspathic litharenites and lithic arkoses with low porosities (7.6% on average) and extremely low permeabilities (0.49 mD on average). A complex diagenetic alteration history of the reservoir caused different kinds of reduction in reservoir porosity. The carbonate cements are sourced from adjacent organic-rich mudstone and precipitated with a higher content near the edges of sandstone units and a lower content at the centres of sandstone units, resulting in two different diagenetic evolution paths. The analysis of porosity evolution history and hydrocarbon emplacement produced the following conclusions: (1) during the eodiagenesis period, mechanical compaction reduced the primary porosity dramatically from 40 to 19%; and (2) during the mesodiagenesis period, the first-phase oil charged the reservoir (porosity ranging from 14 to 19%) as bitumen along detrital grains forming a preferential pathway for subsequent oil emplacements. In the second-phase of oil charge, the reservoir porosity ranged from 9 to 14% limiting water–rock reactions. During the third-phase of oil charge, porosity of the reservoir remained at 9%. In general, the densification period (with a porosity close to 10%) of the reservoir occurs at the same time as the major oil emplacement and may be an explanation for the low oil saturation of the Chang 8 tight sandstone.  相似文献   

高能电子爆发与绕月卫星表面电位大幅下降的联动效应   总被引：2，自引：0，他引：2       下载免费PDF全文

王馨悦  张爱兵  荆涛  H. Reme  孔令高  张珅毅  李春来 《地球物理学报》2016,59(10):3533-3542

"嫦娥"一号、二号绕月飞行经历地球磁尾边界层区域时,分别在2007年11月26日—2008年2月5日和2010年10月3日—2011年2月28日,发现了15次月球轨道0.1~2 MeV电子急剧增加(Bursts of 0.1~2 MeV Energetic Electrons,BEE),卫星周围等离子体离子加速的现象.统计研究表明,这类现象发生在稳定太阳风和弱行星际磁场条件下,且无显著空间环境扰动事件发生时,离子的加速滞后于高能电子爆发,离子能量的变化与高能电子通量的时间演化正相关,地球磁鞘内侧或边界层过渡区域是该类现象的高发区,离子能量增加时卫星表面电位大幅下降可达负几千伏.为了研究高能电子爆发与绕月卫星表面电位变化的关系及其对月球表面电位的影响,本文用电流平衡法建立绕月卫星和月球表面充电模型,并假设能量电子(2eV~2 MeV)满足幂律谱的分布,模拟急剧增加的能量电子对卫星和月球表面电位的影响.模拟结果表明,能量电子急剧增加使得绕月卫星和月球表面电位大幅下降;能量电子总流量1011 cm-2时,绕月卫星和月球表面充电电位可达负上千伏;月球充电到大的负电位的时间仅为卫星充电时间的1/10.鉴于高能电子急剧增加事件的高发生率(~125次/年),能量电子急剧增加使得绕月卫星表面电位大幅下降的发生率应大于实测等离子体离子加速现象的发生率(~25次/年).  相似文献   

川中安平店-高石梯构造震旦系灯影组流体充注特征及油气成藏过程   总被引：1，自引：0，他引：1  

袁海锋  刘勇  徐昉昊  王国芝  徐国盛 《岩石学报》2014,30(3):727-736

川中地区震旦系灯影组储层时代老、埋藏深,经历了多期构造运动和成藏历史。岩芯观察和显微薄片观察结果表明,震旦系灯影组储层经历了六期流体充注,分别是第一世代沥青→第二世代白云石→第三世代粗晶-巨晶白云石→第四世代粗晶-巨晶白云石→第五世代沥青→第六世代方解石/石英,每期矿物中对应的流体包裹体特征记录了震旦系从早期形成的古油藏被破坏→古油气藏再形成→油裂解气和古气藏形成→水溶气形成→现今气藏形成的成藏事件和完整的成藏过程。第二世代-第四世代矿物形成于深埋过程中,是古油气藏形成期的产物,矿物的Sr、C、O稳定同位素表明向震旦系灯影组充注的流体主要是外源流体,具有从深部向浅部流动运移的特征;第六世代矿物所记录的水溶气的形成,也是震旦系最重要的成藏事件;现今的震旦系灯影组气藏主要是晚白垩世以来的构造隆升导致的水溶气脱溶聚集以及油气藏调整和改造的结果。  相似文献   

铁路栈桥桥墩钢围堰的拆除爆破     

李致宗  宁旭展 《南方国土资源》2001,14(3):43-47

钢围堰内混凝土拆除爆破工程较为鲜见 ,文章介绍了该工程所选取的爆破诸参数以及所采用的施工工艺 ,可供同行参考  相似文献   

利用储层流体包裹体确定鄂尔多斯盆地塔巴庙区块上古生界油气充注期次和时期   总被引：5，自引：1，他引：5  

郭振华  陈红汉  赵彦超  刘建章  陈雷 《现代地质》2007,21(4):712-718,737

流体包裹体是保存在储层中的微小流体样品,包含有丰富的地质信息。通过对鄂尔多斯盆地塔巴庙区块18口井的62块流体包裹体样品进行荧光观察和显微测温,认为该区上古生界地层共发生过6期流体活动,均与油气成藏有关,并以第二期—第六期的天然气充注为主。结合埋藏史分析可知,油气成藏分别发生在距今190～150Ma的早侏罗世中期—中侏罗世晚期,150～124Ma的中侏罗世晚期—早白垩世早期,124～101Ma的早白垩世早期—早白垩世中期,101～86Ma的早白垩世中期—早白垩世中末期和86～70Ma的早白垩世中末期—早白垩世末期。其中,早侏罗世中期—中侏罗世晚期为油气充注的初始阶段,中侏罗世晚期—早白垩世早期为轻质油的主要成藏时期,中侏罗世晚期至早白垩世末为研究区内目的层天然气的主要成藏时期。  相似文献